Gamma rays from the nucleus have been observed, establishing the rotational ground state band up to the state at 6.994 MeV excitation energy. The experimental Coulomb energy differences, obtained by comparison with the isobaric analog states in its mirror , confirm the qualitative interpretation of the backbending patterns in terms of successive alignments of proton and neutron pairs. A quantitative agreement with experiment has been achieved by exact shell model calculations, incorporating the differences in radii along the yrast bands, and properly renormalizing the Coulomb matrix elements in the model space.
Excited states have been studied in following the fusion-evaporation reaction at 60 MeV using the Ge-detector array GASP. A comparison with the mirror nucleus shows two remarkable features: (i) A surprisingly large energy difference for the states, in which the hitherto overlooked electromagnetic spin-orbit term is shown to play a major role, and (ii) a very different decay pattern for the states, which provides direct evidence of isospin mixing.
The neutron-rich cobalt isotopes up to A=67 have been studied through multinucleon transfer reactions by bombarding a 238U target with a 460-MeV 70Zn beam. Unambiguous identification of prompt $\gamma${} rays belonging to each nucleus has been achieved using coincidence relationships with the ions detected in a high-acceptance magnetic spectrometer. The new data are discussed in terms of the systematics of the cobalt isotopes and interpreted with large-scale shell-model calculations in the fpgd model space. In particular, very different shapes can be described in 67Co, at the edge of the island of inversion at N=40, where a low-lying highly deformed band coexists with a spherical structure.
Following the heavy-ion fusion-evaporation reaction at 95 MeV beam energy the lifetimes of analogue states in the mirror nuclei and have been measured using the Cologne plunger device coupled to the GASP -ray spectrometer. The deduced values afford a unique opportunity to probe isoscalar and isovector polarization charges and to derive effective proton and neutron charges, and , in the shell. A comparison between the experimental results and several different large-scale shell-model calculations yields and .